Astrophysical uncertainties on the local dark matter distribution and direct detection experiments

The differential event rate in weakly interacting massive particle (WIMP) direct detection experiments depends on the local dark matter density and velocity distribution. Accurate modelling of the local dark matter distribution is therefore required to obtain reliable constraints on the WIMP particl...

Full description

Bibliographic Details
Main Author: Green, Anne M.
Format: Article
Published: IOP Publishing 2017
Online Access:https://eprints.nottingham.ac.uk/43779/
_version_ 1848796766722326528
author Green, Anne M.
author_facet Green, Anne M.
author_sort Green, Anne M.
building Nottingham Research Data Repository
collection Online Access
description The differential event rate in weakly interacting massive particle (WIMP) direct detection experiments depends on the local dark matter density and velocity distribution. Accurate modelling of the local dark matter distribution is therefore required to obtain reliable constraints on the WIMP particle physics properties. Data analyses typically use a simple standard halo model which might not be a good approximation to the real Milky Way (MW) halo. We review observational determinations of the local dark matter density, circular speed and escape speed and also studies of the local dark matter distribution in simulated MW-like galaxies. We discuss the effects of the uncertainties in these quantities on the energy spectrum and its time and direction dependence. Finally, we conclude with an overview of various methods for handling these astrophysical uncertainties.
first_indexed 2025-11-14T19:53:12Z
format Article
id nottingham-43779
institution University of Nottingham Malaysia Campus
institution_category Local University
last_indexed 2025-11-14T19:53:12Z
publishDate 2017
publisher IOP Publishing
recordtype eprints
repository_type Digital Repository
spelling nottingham-437792020-05-04T18:51:48Z https://eprints.nottingham.ac.uk/43779/ Astrophysical uncertainties on the local dark matter distribution and direct detection experiments Green, Anne M. The differential event rate in weakly interacting massive particle (WIMP) direct detection experiments depends on the local dark matter density and velocity distribution. Accurate modelling of the local dark matter distribution is therefore required to obtain reliable constraints on the WIMP particle physics properties. Data analyses typically use a simple standard halo model which might not be a good approximation to the real Milky Way (MW) halo. We review observational determinations of the local dark matter density, circular speed and escape speed and also studies of the local dark matter distribution in simulated MW-like galaxies. We discuss the effects of the uncertainties in these quantities on the energy spectrum and its time and direction dependence. Finally, we conclude with an overview of various methods for handling these astrophysical uncertainties. IOP Publishing 2017-06-26 Article PeerReviewed Green, Anne M. (2017) Astrophysical uncertainties on the local dark matter distribution and direct detection experiments. Journal of Physics G: Nuclear and Particle Physics, 44 (8). 084001. ISSN 1361-6471 http://iopscience.iop.org/article/10.1088/1361-6471/aa7819/meta doi:10.1088/1361-6471/aa7819 doi:10.1088/1361-6471/aa7819
spellingShingle Green, Anne M.
Astrophysical uncertainties on the local dark matter distribution and direct detection experiments
title Astrophysical uncertainties on the local dark matter distribution and direct detection experiments
title_full Astrophysical uncertainties on the local dark matter distribution and direct detection experiments
title_fullStr Astrophysical uncertainties on the local dark matter distribution and direct detection experiments
title_full_unstemmed Astrophysical uncertainties on the local dark matter distribution and direct detection experiments
title_short Astrophysical uncertainties on the local dark matter distribution and direct detection experiments
title_sort astrophysical uncertainties on the local dark matter distribution and direct detection experiments
url https://eprints.nottingham.ac.uk/43779/
https://eprints.nottingham.ac.uk/43779/
https://eprints.nottingham.ac.uk/43779/